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  Gas kinetics of galactic disk. Dark matter is not required to explain rotation curves of S-type galaxies

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Referee this paper: doi: 10.31219/osf.io/t6754 by Anton A. Lipovka

Please use comments to point to previous work in this direction, and reviews to referee the accuracy of the paper. Feel free to edit this submission to summarise the paper (just click on edit, your summary will then appear under the horizontal line)

(Is this your paper?)

requested Aug 16, 2021 by Dilaton (6240 points)
submission not yet summarized
paper authored May 4, 2021 to astro-ph by Anton_Lipovka, 
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